| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 721586 | IFAC Proceedings Volumes | 2007 | 6 Pages |
Abstract
LISA and the next generation of space-based laser interferometers require gravitational reference sensors (GRS) to provide distance measurements with picometer precision. To meet this goal, we describe a stand-alone GRS structure that has high sensitivity and easy integration with a satellite. The stand-alone GRS integrates balanced optical probing of the proof-mass position in its housing, and provides a correlated reference surface to an independent external interferometer. The use of optical sensing allows for a large gap between the proof-mass and housing, which is the best way to reduce many proof-mass disturbances.
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Physical Sciences and Engineering
Engineering
Computational Mechanics
